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Part of a WEAVE fibre configuration

Part of the WEAVE focal plane showing optical fibres positioned on a set of targets in the telescope focal plane.

Prof Gavin Dalton

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Extremely Large Telescope
Gavin.Dalton@physics.ox.ac.uk
  • About
  • Research
  • Publications

The Subaru FMOS Galaxy Redshift Survey (FastSound): The Mass-Metallicity Relation and the Fundamental Metallicity Relation at z ∼ 1.4

MULTI-OBJECT SPECTROSCOPY IN THE NEXT DECADE: BIG QUESTIONS, LARGE SURVEYS, AND WIDE FIELDS 507 (2016) 355-360

Authors:

Kiyoto Yabe, Kouji Ohta, Masayuki Akiyama, Naoyuki Tamura, Fumihide Iwamuro, Tomonori Totani, Gavin Dalton, Andrew Bunker
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Towards an Integrated Model of the WEAVE Performance

MULTI-OBJECT SPECTROSCOPY IN THE NEXT DECADE: BIG QUESTIONS, LARGE SURVEYS, AND WIDE FIELDS 507 (2016) 121-124

Authors:

Sun Jeong Ham, Gavin Dalton
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Verification of Commercial Motor Performance for WEAVE at the William Herschel Telescope

MULTI-OBJECT SPECTROSCOPY IN THE NEXT DECADE: BIG QUESTIONS, LARGE SURVEYS, AND WIDE FIELDS 507 (2016) 117-120

Authors:

James Gilbert, Gavin Dalton, Ian Lewis
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WEAVE: The Next Generation Spectroscopy Facility for the WHT

MULTI-OBJECT SPECTROSCOPY IN THE NEXT DECADE: BIG QUESTIONS, LARGE SURVEYS, AND WIDE FIELDS 507 (2016) 97-102
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The Subaru FMOS Galaxy Redshift Survey (FastSound). III. The mass–metallicity relation and the fundamental metallicity relation at z ∼ 1.4*

Publications of the Astronomical Society of Japan Oxford University Press (OUP) 67:6 (2015) 102

Authors:

Kiyoto Yabe, Kouji Ohta, Masayuki Akiyama, Andrew Bunker, Gavin Dalton, Richard Ellis, Karl Glazebrook, Tomotsugu Goto, Masatoshi Imanishi, Fumihide Iwamuro, Hiroyuki Okada, Ikkoh Shimizu, Naruhisa Takato, Naoyuki Tamura, Motonari Tonegawa, Tomonori Totani
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